logo kso logo uni graz

20220411 - Filament data for 11 UTC
Available data for 20220411: »05 UTC   »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC   »15 UTC  
Click on image to open sensitive map! 
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1005 1870 (N48E39 L=220)   752     79        3 ( 969/1835-1047/1892)  45.0 E42-E35 N44-N51
      2  916 1814 (N39E39 L=220)   814    105        0 ( 893/1758- 946/1862) -51.3 E43-E33 N34-N44
      3 1254 1568 (N33E03 L=256)   790    142        2 (1227/1497-1282/1638) -70.0 E05-W00 N27-N38
      4 1453 1549 (N39W11 L=270)   881    180        2 (1381/1481-1502/1602) -18.4 W04-W16 N35-N41
      5 1546 1357 (N29W22 L=281)   478    117        1 (1513/1303-1585/1404) -23.2 W19-W26 N25-N31
      6  593 1132 (S11E28 L=231)   229     72        0 ( 559/1104- 614/1153) -14.0 E30-E26 S12-S10
      7 1631 1092 (N16W34 L=293)   409     45        0 (1598/1070-1658/1116)  21.8 W31-W36 N14-N17
      8 1669 1042 (N14W38 L=297)   477     73        1 (1626/1022-1703/1072)  26.6 W35-W41 N12-N16
      9 1566  834 (S00W37 L=296)   791    182        3 (1517/ 762-1630/ 912)  78.7 W34-W39 S05-N05
     10  821  876 (S20E07 L=251)   263     63        0 ( 792/ 848- 855/ 902)   0.0 E09-E04 S20-S18
     11  891  561 (S36W07 L=266)   689    278        2 ( 839/ 461- 922/ 677) -76.0 W03-W10 S44-S28
     12  701  621 (S38E08 L=251)   260     81        0 ( 676/ 593- 729/ 649)  59.0 E09-E06 S40-S35
     13  757  453 (S48W02 L=261)   328     77        0 ( 719/ 436- 797/ 474)   9.5 E01-W05 S48-S46
     14 1150  344 (S41W36 L=295)   462     90        0 (1110/ 322-1196/ 370)  14.0 W31-W40 S41-S39
     15 1403  336 (S32W54 L=313)   853     81        1 (1350/ 313-1448/ 357)  18.4 W48-W58 S33-S29
Download FITS filament maps as tar archive

» All Filament Data of 20220411 ... 		The tar archive contains filament maps for all processed Hα images with at least quality=1.
The maps contain the values 0 and 1, where 1 is the position of a detected filament.
The header in the FITS files is mostly taken from the corresponding Hα file, so it should be compatible with standard solar software routines.

» Data Policy » KSO Homepage » Astrophysics and Geophysics » University of Graz     Contact